{"paper":{"title":"A Multi-wavelength View of the Star Formation Activity at z~3","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"CFHT), David Elbaz(CEA), Dimitra Rigopoulou (Oxford), Emanuele Daddi(CEA), Georgios E. Magdis(CEA), Glenn E. Morrison (IfA, Ho Seong Hwang (CEA), Mark Dickinson(NOAO), Raphael Gobat (CEA)","submitted_at":"2010-03-30T09:54:58Z","abstract_excerpt":"We present a multi-wavelength, UV-to-radio analysis for a sample of massive (M$_{\\ast}$ $\\sim$ 10$^{10}$ M$_\\odot$) IRAC- and MIPS 24$\\mu$m-detected Lyman Break Galaxies (LBGs) with spectroscopic redshifts z$\\sim$3 in the GOODS-North field (L$_{\\rm UV}$$>1.8\\times$L$^{\\ast}_{z=3}$). For LBGs without individual 24$\\mu$m detections, we employ stacking techniques at 24$\\mu$m, 1.1mm and 1.4GHz, to construct the average UV-to-radio spectral energy distribution and find it to be consistent with that of a Luminous Infrared Galaxy (LIRG) with L$\\rm_{IR}$=4.5$^{+1.1}_{-2.3}$$\\times 10^{11}$ L$_{\\odot}$"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1003.5773","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}